Dark matter · dark energy

Dark Matter–Dark Energy

How could we test a hypothesis about dark matter and dark energy? DMDE designs a test using two fixed particle-injection scenarios. A future calculation would follow their neutrinos, neutron–proton reactions and the formation of helium and deuterium.

Public source checkpoint v0.9.20

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Research status

A working hypothesis and methods/software release, without peer review. No validated production predictions for helium abundance, deuterium abundance or effective neutrino number are supplied.

What the public work reports

A fixed pair of sources

Two byte-frozen, blinded spectral-source payloads share timing and neutrino shapes while differing in amplitude. The source-only analysis describes their differential-response geometry and conditional precision requirements.

A stronger chain of checks

Public validators, schemas and provider contracts cover source shape, timing, transport stepping, nuclear-input consumption and meaningful refinement. A five-process weak-rate audit includes charged-lepton capture and finite-temperature neutron-decay blocking.

Preserved public materials

The provider directory preserves 74 files from the public provider archive byte for byte. The release directory contains the five published artifacts. The frozen release’s source checks do not run neutrino transport or a Big Bang nucleosynthesis calculation.

Numerical controls for the next test

The 1 October 2026 supplement calculates the known missing inverse weak reaction and runs an established program’s ordinary Standard Model control. A separate computational review checks the equations and recorded outputs. These controls help prepare the future particle-injection calculation; they supply no DMDE abundance predictions and are not external peer review.

Checking the source inside a solver

The 2 October 2026 preflight passes the exact frozen source into a candidate solver’s existing neutrino equations, using an explicit entropy normalization and coordinate map and a cutoff set by the actual state time. Twelve checks at fixed states pass. These demonstrate source consumption and normalization, without an evolved transport history. Separate AI-assisted computational reviews retain the failed precision checks; they are not external scientific peer review.

Assumptions and open questions

Three prerequisites still block a physical transport trajectory: adequate momentum grids, a production source step whose consumption can be checked against the intended source before mixing, and consistent plasma thermodynamics. Full-domain source-grid tests fail the declared precision ceiling, the native unsplit derivative fails the pre-mixing source comparison, and two QED formulas violate pressure identities. The isolated corrected QED components do not validate a complete equation of state, collisions or an evolved trajectory.

Production momentum-dependent transport, corrected weak rates, an instrumented Big Bang nucleosynthesis calculation and independent backend replication remain pending. The five exported weak histories do not separately represent the inverse three-body process; the Born-reference audit is not a complete precision treatment. Source-pair identities do not determine the final abundance response. The approximately twenty-parts-per-million example is a conditional design target, not achieved accuracy or a detection. The wider microscopic model and its dark-energy connection need separate derivations and tests.

Read the source materials

The repository documentation is the primary source for this overview.

Archives and citation

Ricardo Maldonado. DMDE Triplepoint + CosmoGate: Five-Channel Weak-Rate Closure and Frozen-Pair Differential-Response Design (v0.9.20). Zenodo, published September 5, 2026. DOI: 10.5281/zenodo.22399940. The September 30 GitHub packaging introduces no new physical results or research version.

The existing v0.9.20 Zenodo archive and its five release files were verified on 2 October 2026. The later GitHub diagnostics preserve this archival version; no new Zenodo release was created.

Overview updated from public documentation and separately reviewed numerical controls and source-adapter diagnostics on 2 October 2026. Consult the cited source version for full statements, qualifications and reuse terms. Author: Ricardo Maldonado.